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Characterization and device performance of (AgCu)(InGa)Se2 absorber layers

Conference ·
OSTI ID:963892

The study of (AgCu)(InGa)Se2 absorber layers is of interest in that Ag-chalcopyrites exhibit both wider bandgaps and lower melting points than their Cu counterparts. (AgCu)(InGa)Se2 absorber layers were deposited over the composition range 0 < Ag/(Ag+Cu) < 1 and 0.3 < Ga/(In+Ga) < 1.0 using a variety of elemental co-evaporation processes. Films were found to be singlephase over the entire composition range, in contrast to prior studies. Devices with Ga content 0.3 < Ga/(In+Ga) <0.5 tolerated Ag incorporation up to Ag/(Ag+Cu) = 0.5 without appreciable performance loss. Ag-containing films with Ga/(In+Ga) = 0.8 showed improved device characteristics over Cu-only control samples, in particular a 30-40% increase in short-circuit current. An absorber layer with composition Ag/(Ag+Cu) = 0.75 and Ga/(In+Ga) = 0.8 yielded a device with VOC = 890 mV, JSC = 20.5mA/cm2, fill factor = 71.3%, and η = 13.0%.

Research Organization:
University of Delaware, Newark, DE
Sponsoring Organization:
USDOE Assistant Secretary for Energy Efficiency and Renewable Energy (EE); USDOE EERE Office of Solar Energy Technology (EE-2A)
DOE Contract Number:
FG36-08GO18019
OSTI ID:
963892
Report Number(s):
DOE/GO/18019-1
Country of Publication:
United States
Language:
English

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